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Short-term variation in the galactic cosmic ray intensity measured with the PAMELA experiment

Munini, R. (author)
Di Felice, V. (author)
Boezio, M. (author)
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Adriani, O. (author)
Barbarino, G. C. (author)
Bazilevskaya, G. A. (author)
Bellotti, R. (author)
Bogomolov, E. A. (author)
Bongi, M. (author)
Bonvicini, V. (author)
Bottai, S. (author)
Bruno, A. (author)
Cafagna, F. (author)
Campana, D. (author)
Carlson, Per (author)
KTH,Partikel- och astropartikelfysik
Casolino, M. (author)
Castellini, G. (author)
De Donato, C. (author)
De Santis, C. (author)
Galper, A. M. (author)
Karelin, A. V. (author)
Koldashov, S. V. (author)
Koldobskiy, S. (author)
Krutkov, S. Y. (author)
Kvashnin, A. N. (author)
Leonov, A. (author)
Malakhov, V. (author)
Marcelli, L. (author)
Martucci, M. (author)
Mayorov, A. G. (author)
Menn, W. (author)
Merge, M. (author)
Mikhailov, V. V. (author)
Mocchiutti, E. (author)
Monaco, A. (author)
Mori, N. (author)
Osteria, G. (author)
Panico, B. (author)
Papini, P. (author)
Pearce, Mark, 1970- (author)
KTH,Partikel- och astropartikelfysik
Picozza, P. (author)
Ricci, M. (author)
Ricciarini, S. B. (author)
Simon, M. (author)
Sparvoli, R. (author)
Spillantini, P. (author)
Stozhkov, Y. I. (author)
Vacchi, A. (author)
Vannuccini, E. (author)
Vasilyev, G. (author)
Voronov, S. A. (author)
Yurkin, Y. T. (author)
Zampa, G. (author)
Zampa, N. (author)
Potgieter, M. S. (author)
Christian, E. C. (author)
De Nolfo, G. A. (author)
Richardson, I. (author)
Ryan, J. M. (author)
Stochaj, S. (author)
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 (creator_code:org_t)
Sissa Medialab Srl, 2017
2017
English.
In: Proceedings of Science. - : Sissa Medialab Srl.
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • New results on the galactic cosmic ray (GCR) short-term intensity variation associated with Forbush decrease and co-rotating interaction regions (CIRs) measured by the PAMELA instrument between November 2006 and March 2007 are presented. Most of the past measurements on Forbush decrease events were carried out with neutron monitor detector. This tecnique allows only indirect detection of the overall GCR intensity over an integrated energy range. For the first time, thanks to the unique features of the PAMELA magnetic spectrometer, the Forbush decrease associated with the December 13th coronal mass ejection (CME) was studied in a wide rigidity range (0.4 - 20 GV) and for different species of GCRs detected directly in space. Using GCR protons, the amplitude and the recovery time of the Forbush decrease were studied for ten rigidity interval with a temporal resolution of one day. For comparison the helium and the electron intensity over time were also studied. The temporal evolution of the helium and proton intensity was found in good agreement while the electrons show, on average, a faster recovery time. This was interpreted as a charge-sign dependence introduced by drift motion experienced by the low rigidity (< 5 GV) GCRs during their propagation through the heliosphere. Moreover a clear 13.5 days cyclical variation was observed in the GCR proton intensity after the Forbush decrease. This phenomena could be interpreted as an effect of prominent structures of compressed plasma in the solar wind, i.e. CIRs, or to the latitudinal gradient due to the crossing of the heliospheric current sheet (HCS). 

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

Cosmology
Helium
Magnetic fields
Rigidity
Coronal mass ejection
Galactic cosmic rays
Heliospheric current sheet
Intensity variations
Latitudinal gradients
Magnetic spectrometers
Prominent structures
Short-term variations
Cosmic rays

Publication and Content Type

ref (subject category)
kon (subject category)

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